Light Superpartners at Hadron Colliders

Details Light Superpartners at Hadron Colliders Light Superpartners at Hadron Colliders

2005-10-19

arxiv.org/abs/hep-ph/0510252v2

Int.J.Mod.Phys.A21:5221-5240,2006

Physics

High Energy Physics

High Energy Physics - Phenomenology

18 pages, LaTeX, uses axodraw.sty

Scientific paper

10.1142/S0217751X06034008

Uncertainties of the MSSM predictions are due to an unknown SUSY breaking mechanism. To reduce these uncertainties, one usually imposes constraints on the MSSM parameter space. Recently, two new constraints became available, both from astrophysics: WMAP precise measurement of the amount of the Dark Matter in the Universe and EGRET data on an excess in diffuse gamma ray flux. Being interpreted as a manifestation of supersymmetry these data lead to severe constraints on parameter space and single out a very restricted area. The key feature of this area is the splitting of light gauginos from heavy squarks and sleptons. We study the phenomenological properties of this scenario, in particular, the cross-sections of superparticle production, their decay patterns and signatures for observation at hadron colliders, Tevatron and LHC. We found that weakly interacting particles in this area are very light so that the cross-sections may reach fractions of a pb with jets and/or leptons as final states accompanied by missing energy taken away by light neutralino with a mass around 100 GeV.

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